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Does mass increase in SR mean higher gravity in GR? |
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| Dec23-04, 10:35 PM | #1 |
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Does mass increase in SR mean higher gravity in GR?
It has been years since I have thought of relativity, but I came across a book by Jerome Drexler in which he attempts to support his view that ultra high energy protons (cosmic rays) are what dark matter is all about in the galactic halos. In spite of the fact that it seems to me these protons would interact and emit radiation (hence be detectable), he argues that the mysterious gravitational influences from these photons is due to the relativistic mass increase due to their high velocities. This doesn't make sense to me. If this were true, it seems like I could tie a ball to a string and twirl it around fast enough to create enough relativistic mass to bring the moon crashing down to Earth! Obviously this is crazy, but I think the idea is the same. Does anyone have any explanations or thoughts as to what gravitational effects fast moving objects would have. It does not make sense to me that they would have any at all.
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| Dec24-04, 12:57 AM | #2 |
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AM2 |
| Dec24-04, 02:48 AM | #3 |
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Incorrect. The energy used to accelerate an object must be subtracted from the apparent relativistic mass gain. The net effect is zero.
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| Dec24-04, 03:44 AM | #4 |
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Does mass increase in SR mean higher gravity in GR?They agreed qualitatively, but not quantitatively :-(. Somoene else here has worked on the problem, too, but I don't really believe his answer either. I do have a paper which works out the results for low velocity, though. Qualtiatively, though, the field will increase in the transverse direction, i.e if X marks the "spot" (particle). X----> direction of motion | | \/ max field There will also be a "magnetic" like field that will affect moving particles (but it won't matter to the force on a stationary particle) this is known as "frame dragging", or also as gravitomagnetism. For the electric field of a relativistically moving charge (which will be generally similar, but not exactly the same as the gravitational result) see java applet for this java applet, note that the field strength is equal to the density of the field lines. and if you'd rather see the equations, this link has them equation form |
| Dec24-04, 09:28 AM | #5 |
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AM2 |
| Dec25-04, 04:39 AM | #6 |
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Pete |
| Dec25-04, 05:02 AM | #7 |
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No object can change speed without being accelerated. The only relevant factor is the reference frame from which you measure it.
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| Dec25-04, 07:20 AM | #8 |
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However if the person swinging the ball got energy from outside the Earth to swing the ball then the gravitational field of the Earth/ball system would increase. Pete |
| Dec25-04, 10:49 AM | #9 |
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Actually, I would be really happy if someone could give me a good explanation of how kinetic energy works in special relativity.
I mean, if a 1 kg rock hits the earth at 100 m/s, you usually calculate the energy of that collision by using the mass of the rock. Why don't you use the mass of the Earth? Why isn't the Earth moving towards the rock instead? |
| Dec25-04, 01:03 PM | #10 |
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Einstein concluded in one of his papers that a particle's increase in inertial mass due to motion would result in an increase in its gravitational mass As Andrew Mason has said. I don't know of any actual reported experiments however - anyone have a reference on this. It does seem to raise some paradoxical questions- but it also seems that it must follow from the equivalence principle.
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| Dec26-04, 01:40 AM | #11 |
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The gravitational effect, however, is the same in both reference frames. Since gravity is the product of both masses, it doesn't matter which mass the [itex]\gamma[/itex] factor applies to. It is still [itex]F \propto \gamma m M/R^2[/itex] AM |
| Dec26-04, 02:15 AM | #12 |
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Columb's law does not work for relativistically moving charges. Similarly, Newton's law of gravitation will not work for relativistically moving masses. |
| Dec26-04, 02:20 AM | #13 |
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The physically significant quantity in a collision between two masses is the energy in the center-of-mass frame. If a 1kg rock hits the earth at 100m/s, the center of mass frame is essentially that of the Earth. You can acutally work the problem of the rock hitting the earth out in any frame you desire, but the center of mass frame is the simplest, and the most standard. Note that this is why particle accelerators go to the bother of creating anti-protons to slam into protons with an equal and opposite velocity. The energy that counts is the energy in the center-of-mass frame, and much of this energy is lost when a hyper-relativistic particle strikes a stationary target. You get well over double the energy in a "head-on" collision. |
| Dec26-04, 07:49 AM | #14 |
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The active gravitational mass of a moving body is not [itex]\gamma M[/itex], its [itex]\gamma M(1+\beta^2)[/itex]. See - http://www.geocities.com/physics_wor...oving_body.htm Pete |
| Dec26-04, 11:46 AM | #15 |
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I still don't see where you get eq 3a) in your derivation - I was hoping that the paper you cited by Harris would answer this question, but it does not.
Harris ("Analogy between general relativity and electromagnetism .......") gives the formula [tex] m\frac{d^2 x^u}{d \tau^2} + m\Gamma^u{}_{ab}(\frac{dx^a}{d \tau})(\frac{dx^b}{d \tau}) [/tex] his eq 1a), as the formula for deriving "force", which I do believe, at least as long as one is in a coordinate basis (the last point may seem picky, but it was the source of at least some of my earlier difficulties). |
| Dec26-04, 12:34 PM | #16 |
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| Dec26-04, 02:47 PM | #17 |
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I should add, that by applying the above definition, for the metric for Newtonian gravity ([tex] U = - \Phi [/tex])
(1+2U)dx^2 + (1+2U)dy^2 + (1+2U)dz^2 - (1-2U) dt^2 with a 4-velocity [tex] (t,x,y,z) = (\gamma, \beta \gamma, 0, 0) [/tex] [tex]\beta = v/c, \gamma = 1/\sqrt{1-\beta^2}[/tex] I'm getting [tex] \frac{d^2 x}{d \tau^2} = \frac{\frac{\partial U}{\partial x} - 2 \gamma^2 \frac{\partial U}{\partial t}}{1+2U} [/tex] the main concern is the term in the partial of U with repsect to t (as U is not necessarily indpedent of time depending on the coordinate system used). [add] also [tex] \frac{d^2 y}{d \tau^2} = \frac{1+\beta^2}{(1+2U)(1-\beta^2)} \,\frac{\partial U}{\partial y} [/tex] which also didn't seem compatible |
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